The gravity group: Missing pics: Michael Horbatsch, Alex Dietz, Cody Arceneaux…

Slides:



Advertisements
Similar presentations
Low scale gravity black holes at LHC
Advertisements

Physics 55 Friday, December 2, Quiz 7 (last quiz) 2.Relativistic mass, momentum, energy 3.Introduction to General Relativity 4.Einstein’s equivalence.
Dark Energy and Quantum Gravity Dark Energy and Quantum Gravity Enikő Regős Enikő Regős.
SIKKIM MANIPAL INSTITUTE OF TECHNOLOGY (SMIT) IN INDIA-CMS Gobinda C Mishra & Raman K Jha SMIT September 27-28, 2007 India-CMS Meeting, Delhi University,
Galactic Super Massive Binary Black Hole Mergers Galactic Super Massive Binary Black Hole Mergers Dr. Peter Berczik Astronomisches Rechen-Institut (ARI),
EMMI - Hot Matter Aug 2010 | Vienna, Austria Colliding black holes Vitor Cardoso (CENTRA/IST & Olemiss)  PRL101:161101,2008; PRL103:131102,2009;
What is gravity?. We all know about gravity We see and experience its effects every day Not just on Earth… DigitalImages/1995/1995_02395L.jpg.
Astrophysical tests of general relativity in the strong-field regime Emanuele Berti, University of Mississippi/Caltech Texas Symposium, São Paulo, Dec.
Energy extraction from black holes Vitor Cardoso (CENTRA/IST & Olemiss) BHs Dec 2011 | Aveiro, Portugal Credit: ESO/MPE (2010)
Dark Energy and Void Evolution Dark Energy and Void Evolution Enikő Regős Enikő Regős.
Edmund Bertschinger MIT Department of Physics and Kavli Institute for Astrophysics and Space Research General Relativity and Applications 2. Dynamics of.
July 7, 2008SLAC Annual Program ReviewPage 1 Particle Astrophysics and Cosmology Theoretical Research Overview R. Blandford KIPAC Director, PPA Assistant.
Gravity with the SKA Michael Kramer Jodrell Bank Observatory University of Manchester With Don Backer, Jim Cordes, Simon Johnston, Joe Lazio and Ben Stappers.
The 2d gravity coupled to a dilaton field with the action This action ( CGHS ) arises in a low-energy asymptotic of string theory models and in certain.
1 Amaldi 5 GWIC Report by B Barish, chair. 2 GWIC gravitational wave international committee  International Union of Physics and Applied Physics (IUPAP)
Teória relativity začiatok alebo koniec fyziky.
Particle Physics Professor Kay Kinoshita University of Cincinnati.
Gravitational Waves (& Gravitons ?)
1 Yasushi Mino Theoretical AstroPhysics Including Relativity (TAPIR), CalTech Index 1: Introduction: LISA project 2: MiSaTaQuWa.
Key Open Problems in Black Hole Physics and Gravitation Theory Today (A personal perspective!) Pankaj S. Joshi.
Case Western Reserve University May 19, Imaging Black Holes Testing theory of gas accretion:Testing theory of gas accretion: disks, jets Testing.
Why we analyze data Lee Samuel Finn Center for Gravitational Wave Physics.
Elcio Abdalla Perturbations around Black Hole solutions.
1 FK7003 Elementary Particle Physics David Milstead A4:1021 tel: /
Modern Physics Modern Physics Global Mechanics Global Mechanics Astrophysics Astrophysics Cosmology and The Little Bang Cosmology and The Little Bang.
Clifford Will Washington University John Archibald Wheeler International School on Astrophysical Relativity Theoretical Foundations of Gravitational-Wave.
Marco Cavaglià –University of Mississippi - MIT, July 22-26, 2007 LSC in Mississippi: A proposal of membership Marco Cavaglià on behalf of the UMGr 2 LIGO-G Z.
Objective of numerical relativity is to develop simulation code and relating computing tools to solve problems of general relativity and relativistic astrophysics.
Einstein’s elusive waves
Yi-Zen Chu BCCS Case Western Reserve University 9 December 2008 The n-body problem in General Relativity from perturbative field theory arXiv:
International Workshop on Astronomical X-Ray Optics Fingerprints of Superspinars in Astrophysical Phenomena Zdeněk Stuchlík and Jan Schee Institute of.
ASTR 567: Observational Techniques in Astronomy. ASTR 567: Grading Scheme Start of lecture quizzes………………….. 10% Homeworks……………………………………..25% Highest of.
Emanuele Berti Aristotle University of Thessaloniki In collaboration with: Kostas Kokkotas, Vitor Cardoso, Hisashi Onozawa Suggested.
Self-Force and the m-mode regularization scheme Sam Dolan (with Leor Barack) University of Southampton BriXGrav, Dublin 2010.
String Theory Mihir John What are the most basic constituents that make up the universe around us?
Searching for Gravitational Waves with LIGO: A New Window on The Universe Duncan Brown Syracuse University RIT Physics Colloquium November 19, 2007 LIGO-G Z.
Quantum Steering in the Gaussian World Ioannis Kogias, A. Lee, S. Ragy and G. Adesso University of Nottingham To appear on arXiv: [quant-ph]
Theoretical Issues in Astro Particle Physics J.W. van Holten April 26, 2004.
Composition Until 30 years ago, we thought all matter was “baryonic” matter (protons, neutrons, electrons). Now: 4.6% is baryonic matter 95% is non-baryonic.
ExDiP Nov 2010 | KEK, Japan Instabilities of (very) compact objects Vitor Cardoso (CENTRA/IST & Olemiss) 
Motions of Self-Gravitating bodies to the Second Post- Newtonian Order of General Relativity.
Dragan Slavkov Hajdukovic
New Worlds In black hole physics supports this project   Vítor Cardoso (CENTRA/IST) NewWorlds, Lisbon 2012  More at
Gravitational Physics in Thessaloniki (AUTH) EUROPEAN NETWORK GROUP Kostas Kokkotas Nikolaos Stergioulas Johannes Ruoff (Post-doc, Marie-Curie Fellow)
Low scale gravity black holes at LHC Enikő Regős ( CERN )
1 Yasushi Mino ( 蓑 泰 志 ) WUGRAV, Washington University at St. Louis Index 1: Introduction 2: Self-force in a Linear Perturbation.
Mike Cruise University of Birmingham Searching for the fifth dimension using gravitational waves.
Dark Matter and Energy What are our eyes missing?.
Detector R&D through the NSF PHY division. Jim Shank/Jim Whitmore, NSF CPAD Meeting Arlington, TX 5-7 October, 2015.
Soichiro Isoyama Collaborators : Norichika Sago, Ryuichi Fujita, and Takahiro Tanaka The gravitational wave from an EMRI binary Influence of the beyond.
GW – the first GW detection ! Is it a start of GW astronomy ? If “yes” then which ? «Счастлив, кто посетил сей мир в его минуты роковые !...» Ф.Тютчев.
University of Arizona D IMITRIOS P SALTIS Tests of General Relativity with the SKA.
Statements of the interest in LCGT data analysis Ping Xi Shanghai United Center for Astrophysics (SUCA), Shanghai Normal University.
Mike Cruise University of Birmingham Searches for very high frequency gravitational waves.
LISA Laser Interferometer Space Antenna: The Mission Mike Cruise For the LISA Team.
2. April 2007J.Wicht : Dark Matter2 Outline ● Three lecturers spoke about Dark Matter : – John Ellis, CMB and the Early Universe – Felix Mirabel, High-Energy.
 The universe is everything throughout space.  The universe is constantly changing. It is being created and destroyed all of the time.  There are many.
Zdeněk Stuchlík, Gabriel Török, Petr Slaný Multi-resonant models of quasi-periodic oscillations Institute of Physics, Faculty of Philosophy and Science,
Gravitational wave sources
The Quest for Gravitational Waves: a global strategy
The search for those elusive gravitational waves
Elementary Particle Physics
Theoretical Particle Physics Group (TPP)
Formal Theory Nick Evans (University of Southampton)
Experimental tests of the no-hair theorems of black holes
Solutions of black hole interior, information paradox and the shape of singularities Haolin Lu.
Gravitational wave detection and the quantum limit
The Laser Interferometer Gravitational-wave Observatory
GRAVITATIONAL COLLAPSE, BLACK HOLES AND NAKED SINGULARITIES
LIGO/Virgo Data Analysis and Modified Gravity (MOG) Black Holes
Presentation transcript:

The gravity group: Missing pics: Michael Horbatsch, Alex Dietz, Cody Arceneaux…

Black holes and compact binaries: astrophysics and high-energy physics Emanuele Berti, University of Mississippi/Caltech University of Mississippi, 9/7/2010

Work at Ole Miss (since Jan 2009): 30+ papers 1)Black hole perturbation theory and quasinormal modes Main applications: a) Astrophysics (tests of the no-hair theorem) b) Gauge-gravity duality 110-page review (arXiv: , with Cardoso & Starinets) Critical phenomena: Lyapunov exponents Quantum mechanical scattering: Breit-Wigner resonances Green’s functions techniques: quasinormal mode excitation 2)Numerical relativity and relativistic black hole collisions Head-on collisions (E<14%, no naked singularities; PRL) Grazing collisions (E 0.95; PRL) Astrophysical rotating BHs are not particle accelerators (PRL) Semianalytic study: zero-frequency limit, point particles Superkicks for ultrarelativistic collisions

Work at Ole Miss (since Jan 2009): 30+ papers 3)Black hole astrophysics Spin-orbit resonances: implications for recoil distribution Compact binary rates for advanced detectors – workshop! eLISA Science Taskforce Massive black hole cosmic history Eccentric binaries 4)Astrophysical tests of strong-field gravity Stars in extended gravity theories, spontaneous scalarization Gravastars and superspinars Graviton mass bounds with compact binaries Massive scalar fields: a) Tests in the Solar System/with gravitational waves b) Superradiance and floating orbits (PRL) c) Bosenovas and limits on the photon mass

Support: As PI or Co-PI: NSF Grant PHY ($150k, ) NSF CAREER Grant PHY ($460k, ) NSF Grant PHY ( , 6.5million CPU hours) with U.Sperhake (Cambridge), V.Cardoso (Lisbon), F.Pretorius (Princeton) European Union FP7 IRSES (318k euros, ) ”International Research Staff Exchange Scheme”; E.Berti (UM), V.Cardoso (Lisbon), L.Crispino (Belém), L.Gualtieri (Rome), C.Herdeiro (Aveiro), U.Sperhake (Cambridge) Pending: GAANN proposal to fund 4/5 graduate students every year As collaborator: SFB Project on Advanced LIGO/Virgo Rates (10k euros, 2012) CERN/FP/123593/2011 FCT PTDC/FIS/098025/2008 FCT PTDC/CTE-AST/098032/2008

People at Ole Miss

Starting September 2012: Michael Horbatsch (postdoc), Davide Gerosa (Master student in Milan)